Polarization Characteristics of Io-related Jupiter 18 MHz Radio Emissions

Details Polarization Characteristics of Io-related Jupiter 18 MHz Radio Emissions Polarization Characteristics of Io-related Jupiter 18 MHz Radio Emissions

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm23b1602h&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM23B-1602

Astronomy and Astrophysics

Astronomy

[5737] Planetary Sciences: Fluid Planets / Magnetospheres, [6954] Radio Science / Radio Astronomy

Scientific paper

Jupiter decametric radio emissions at 18 MHz were recorded with a crossed dipole polarimeter during 2000 - 2003 at the University of Florida Radio Observatory (UFRO). These data were recorded at a rate of two samples per second and the axial ratios (i.e. the percentage of circular polarization) were calculated for several Io-related radio emission events. Using this good time resolution data, we explore how the axial ratio evolves with time in each event and how Io-related emissions from the same source compare. We present a summary of axial ratio values for all Io-related radio sources.

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